In this article, we want to explore and delve into IC 1337, a topic that has captured the attention and interest of many people in recent times. IC 1337 has generated debate, research and curiosity in different areas, and its relevance is undeniable. Along these lines, we will delve into the details and particularities of IC 1337, analyzing its impact, its ramifications and its importance today. From different perspectives and approaches, we will seek to understand the extent to which IC 1337 shapes our world and our experiences, offering a detailed and comprehensive view of this fascinating topic.
IC 1337 | |
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![]() IC 1337 by SDSS | |
Observation data (J2000 epoch) | |
Constellation | Capricornus |
Right ascension | 20h 56m 52.742s [1] |
Declination | −16° 35′ 08.88″[1] |
Redshift | 0.030741[2] |
Heliocentric radial velocity | 9216 ± 10 km/s[2] |
Distance | ~420 Mly (129 Mpc)[2] |
Apparent magnitude (V) | 14.5[2] |
Characteristics | |
Type | SAB(r)b pec[2] |
Apparent size (V) | 1.2' x 1.1'[2] |
Other designations | |
MCG-03-53-012, PGC 65760[2] |
IC 1337 is an intermediate spiral galaxy in the constellation Capricornus. The galaxy is located close to the celestial equator. It was discovered by Stéphane Javelle on July 22, 1892. [3]
One supernova has been observed in IC 1337: SN 2019gwl (type II, mag. 19.15).[4]